Solar and Stellar Interiors
Asteroseismology of Red Giants, RV Jitter, Mass Loss, Chemically Peculiar Stars.
Education and employment:
2019.04 - present, Postdoctoral Scientist: Max Planck Institute for Solar System Research, Germany
2015-09 - 2019.03, PhD in Astrophysics: Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, Australia
2012.09 - 2015.07, MSc in Astrophysics: Department of Astronomy, Beijing Normal University, China
2008.09 - 2012.07, MSc in Physics: School of Physics and Astronomy, Yunnan University, China
- Jie Yu et al., submitted. Asteroseismology of luminous red giants with Kepler II: interplay between mass loss, pulsations, and radiation.
- Jie Yu et al., 2020, MNRAS, 493, 1388. Asteroseismology of luminous red giants with Kepler I: Long Period Variables with radial and non-radial modes.
- Jie Yu et al., 2018, MNRAS, 480, L48. Predicting radial-velocity jitter induced by stellar oscillations based on Kepler data.
- Jie Yu et al.. 2018, ApJS, 236, 42. Asteroseismology of 16000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii.
- Jie Yu et al., 2016, MNRAS, 463, 1297. Asteroseismology of 1523 misclassified red giants using Kepler data.